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Detailed Description of J/A+AS/131/141
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Individual files can be fetched (via http) from
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The catalogue can be queried from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+AS/131/141
This standardized document follows the rules of the Standard Description for Astronomical Catalogues. For those having to work on this catalogue using FORTRAN programs, this ReadMe file can be transformed into a f77-compliant program which reads the files making up this catalogue, in two versions: either a f77 program loading whole files into arrays, or a f77-program reading each data file line by line.
J/A+AS/131/141 Stark broadening of O VII and Mg XI (Dimitrijevic+ 1998)
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Stark broadening of spectral lines of multicharged ions of astrophysical
interest. XX: O VII and Mg XI spectral lines
Dimitrijevic M.S., Sahal-Brechot S.
<Astron. Astrophys. Suppl. Ser. 131, 141 (1998)>
=1998A&AS..131..141D (SIMBAD/NED BibCode)
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ADC_Keywords: Atomic physics
Keywords: atomic data - line profiles - plasma
Abstract:
Using a semiclassical perturbation approach, we have calculated
electron-, proton-, and He III-impact line widths and shifts for 14 O
VII and 18 Mg XI multiplets. For O VII, perturber densities are
1017-1023cm-3 and temperatures T=100000-2000000K. For Mg XI,
perturber densities are 1018-1024cm-3 and temperatures
T=500000-5000000K. For lower perturber densities, the Stark broadening
parameters are proportional to the perturber density.
File Summary:
FileName Lrecl Records Explanations
× ReadMe 80 . This file
× table1.dat 123 336 Stark broadening parameters due to e-, p- and
He III-impacts for O VII
× table2.dat 123 468 Stark broadening parameters due to e-, p- and
He III-impacts for Mg XI
See also:
VI/98 : Stark broadening of H lines (Stehle+, 1999)
Stark broadening of other elements (Dimitrijevic, Sahal-Brechot, Popovic)
J/A+AS/105/243 : BeI lines (Dimitrijevic+ 1994)
J/A+AS/105/245 : Al XI and Si XII (Dimitrijevic+ 1994)
J/A+AS/107/349 : Ne VIII and Na IX (Dimitrijevic+ 1994)
J/A+AS/109/551 : OIV and OV (Dimitrijevic+ 1995)
J/A+AS/115/351 : C V and P V (Dimitrijevic+, 1996)
J/A+AS/116/359 : Xe II lines (Popovic+, 1996)
J/A+AS/117/127 : solar Mg I lines (Dimitrijevic+, 1996)
J/A+AS/119/369 : Be III and B III (Dimitrijevic+, 1996)
J/A+AS/119/529 : Sr I spectral lines (Dimitrijevic+, 1996)
J/A+AS/120/373 : Sc II, Y II and Zr II Stark width (Popovic+ 1996)
J/A+AS/122/163 : Ba I and Ba II lines (Dimitrijevic+, 1996)
J/A+AS/122/533 : P IV spectral lines (Dimitrijevic+, 1997)
J/A+AS/127/295 : Kr II lines (Popovic+ 1998)
J/A+AS/127/543 : S V lines (Dimitrijevic+ 1998)
J/A+AS/128/203 : Mn, Ga & Ge multiplets (Popovic+ 1998)
J/A+AS/128/359 : Ca IX and Ca X lines (Dimitrijevic+ 1998)
J/A+AS/129/155 : Si XI and Si XIII lines (Dimitrijevic+ 1998)
J/A+AS/130/539 : Na X (Dimitrijevic+ 1998)
J/A+AS/131/143 : Sc X, Sc XI, Ti XI and Ti XII (Dimitrijevic+ 1998)
J/A+AS/133/227 : K VIII and K IX (Dimitrijevic+ 1998)
J/A+AS/140/191 : Ca I (Dimitrijevic+ 1999)
J/A+AS/140/193 : Zn I (Dimitrijevic+ 1999)
J/A+A/400/791 : Be III (Dimitrijevic+ 2003)
J/A+A/417/375 : Cd III (Milovanovic+, 2004)
J/A+A/423/397 : Si V (Ben Nessib+, 2004)
J/A+A/425/1147 : Ga I (Dimitrijevic+, 2004)
Byte-by-byte Description of file: table1.dat table2.dat
Bytes Format Units Label Explanations
1- 7 E7.2 cm-3 N Perturber density
9- 13 A5 --- El Element
15- 20 A6 --- Tr Transition
24- 30 F7.1 0.1nm lambda Wavelength
33- 40 E8.2 0.1nm/cm3 C Parameter C (1)
43- 50 F8.0 K T Temperature
52 A1 --- n_We [*] Validity of impact approximation (4)
53- 61 E9.3 0.1nm We FWHM for electron impacts (2)
63 A1 --- n_de [*] Validity of impact approximation (4)
64- 73 E10.3 0.1nm de Shift for electron impacts (3)
76 A1 --- n_Wp [*] Validity of impact approximation (4)
77- 85 E9.3 0.1nm Wp FWHM for proton impacts (2) (5)
88 A1 --- n_dp [*] Validity of impact approximation (4)
89- 98 E10.3 0.1nm dp Shift for proton impacts (3) (5)
101 A1 --- n_WHe++ [*] Validity of impact approximation (4)
102-110 E9.3 0.1nm WHe++ FWHM for He III-impacts (2)
113 A1 --- n_dHe++ [*] Validity of impact approximation (4)
114-123 E10.3 0.1nm dHe++ Shift for He III-impacts (3)
Note (1): C/FWHM gives an estimate of the maximum perturber density for which
the line may be treated as isolated and tabulated data may be used
Note (2): FWHM denotes Full Width at Half Maximum
Note (3): A positive (resp. negative) shift is towards the red (resp. blue)
Note (4): An asterisk in this column indicates that 0.1<NV<0.5, (V = collision
volume); beware of the fact that the limit of validity of the impact
approximation is attained for the value that follows
Note (5): Values for NV>0.5 are not given, because in this case the impact
approximation is no longer valid
Acknowledgements: Dr Milan Dimitrijevic
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(End) Patricia Bauer [CDS] 05-Feb-1998